ETAP: An Exoplanetary Transit Analyzer Program

dc.contributor.authorDemircan, Osman
dc.contributor.authorBakis, Volkan
dc.date.accessioned2025-01-27T20:27:06Z
dc.date.available2025-01-27T20:27:06Z
dc.date.issued2015
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.descriptionConference on Living Together: Planets, Host Stars and Binaries -- SEP 08-12, 2014 -- Litomysl, CZECH REPUBLIC
dc.description.abstractWe introduce new software for the modeling of exoplanet transit light curves. The technique is based on the aperture cross correlation between the light changes and the diffraction pattern of the apertures representing the eclipsing binary components (Kopal 1977; Kopal & Demircan 1978), where in the present case the eclipsing component is considered to be a transiting exoplanet. The software finds the best parameters including the fractional radii of the exoplanet and the host star, the inclination and eccentricity of the orbit, the longitude of periastron, limb-darkening coefficients of any degree, and the transit time, yielding the lowest chi(2). Parameter uncertainties are calculated with the jackknife method. We compare results for selected exoplanet transit light curves against those available in the literature.
dc.description.sponsorshipSci Org Comm
dc.identifier.endpage364
dc.identifier.isbn978-1-58381-877-0
dc.identifier.isbn978-1-58381-876-3
dc.identifier.startpage362
dc.identifier.urihttps://hdl.handle.net/20.500.12428/22580
dc.identifier.volume496
dc.identifier.wosWOS:000369467900086
dc.identifier.wosqualityN/A
dc.indekslendigikaynakWeb of Science
dc.language.isoen
dc.publisherAstronomical Soc Pacific
dc.relation.ispartofLiving Together: Planets, Host Stars, and Binaries
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectEclipsing Variables
dc.subjectFourier-Analysis
dc.subjectLight Curves
dc.titleETAP: An Exoplanetary Transit Analyzer Program
dc.typeConference Object

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